Erratum: The JCMT BISTRO survey: Magnetic fields associated with a network of filaments in NGC 1333 (Astrophysical Journal (2020) 899 (28) DOI: 10.3847/1538-4357/aba1e2)

Yasuo Doi; Tetsuo Hasegawa; Ray S. Furuya; Simon Coudé; Charles L.H. Hull; Doris Arzoumanian; Pierre Bastien; Michael Chun-Yuan Chen; James Di Francesco; Rachel Friesen; Martin Houde; Shu Ichiro Inutsuka; Steve Mairs; Masafumi Matsumura; Takashi Onaka; Sarah Sadavoy; Yoshito Shimajiri; Mehrnoosh Tahani; Kohji Tomisaka; Chakali Eswaraiah; Patrick M. Koch; Kate Pattle; Chang Won Lee; Motohide Tamura; David Berry; Tao Chung Ching; Jihye Hwang; Woojin Kwon; Archana Soam; Jia Wei Wang; Shih Ping Lai; Keping Qiu; Derek Ward-Thompson; Do Young Byun; Huei Ru Vivien Chen; Wen Ping Chen; Zhiwei Chen; Jungyeon Cho; Minho Choi; Yunhee Choi; Antonio Chrysostomou; Eun Jung Chung; Pham Ngoc Diep; Hao Yuan Duan; Lapo Fanciullo; Jason Fiege; Erica Franzmann; Per Friberg; Gary Fuller; Tim Gledhill; Sarah F. Graves; Jane S. Greaves; Matt J. Griffin; Qilao Gu; Ilseung Han; Jennifer Hatchell; Saeko S. Hayashi; Thiem Hoang; Tsuyoshi Inoue; Kazunari Iwasaki; Il Gyo Jeong; Doug Johnstone; Yoshihiro Kanamori; Ji Hyun Kang; Miju Kang; Sung Ju Kang; Akimasa Kataoka; Koji S. Kawabata; Francisca Kemper; Gwanjeong Kim; Jongsoo Kim; Kee Tae Kim; Kyoung Hee Kim; Mi Ryang Kim; Shinyoung Kim; Jason M. Kirk; Masato I.N. Kobayashi; Vera Konyves; Takayoshi Kusune; Jungmi Kwon; Kevin Lacaille; Chi Yan Law; Chin Fei Lee; Hyeseung Lee; Jeong Eun Lee; Sang Sung Lee; Yong Hee Lee; Dalei Li; Di Li; Hua Bai Li; Hong Li Liu; Junhao Liu; Sheng Yuan Liu; Tie Liu; Ilse De Looze; A. Ran Lyo; Brenda C. Matthews; Gerald H. Moriarty-Schieven; Tetsuya Nagata; Fumitaka Nakamura; Hiroyuki Nakanishi; Nagayoshi Ohashi; Geumsook Park; Harriet Parsons; Nicolas Peretto; Tae Soo Pyo; Lei Qian; Ramprasad Rao; Mark G. Rawlings; Brendan Retter; John Richer; Andrew Rigby; Hiro Saito; Giorgio Savini; Anna M.M. Scaife; Masumichi Seta; Hiroko Shinnaga; Ya Wen Tang; Yusuke Tsukamoto; Serena Viti; Hongchi Wang; Anthony P. Whitworth; Hsi Wei Yen; Hyunju Yoo; Jinghua Yuan; Hyeong Sik Yun; Tetsuya Zenko; Chuan Peng Zhang; Guoyin Zhang; Yapeng Zhang; Jianjun Zhou; Lei Zhu; Philippe André; C. Darren Dowell; Stewart P.S. Eyres; Sam Falle; Sven Van Loo; Jean François Robitaille

doi:10.3847/1538-4357/abf2b3

Erratum: The JCMT BISTRO survey: Magnetic fields associated with a network of filaments in NGC 1333 (Astrophysical Journal (2020) 899 (28) DOI: 10.3847/1538-4357/aba1e2)

Yasuo Doi, Tetsuo Hasegawa, Ray S. Furuya, Simon Coudé, Charles L.H. Hull, Doris Arzoumanian, Pierre Bastien, Michael Chun-Yuan Chen, James Di Francesco, Rachel Friesen, Martin Houde, Shu Ichiro Inutsuka, Steve Mairs, Masafumi Matsumura, Takashi Onaka, Sarah Sadavoy, Yoshito Shimajiri, Mehrnoosh Tahani, Kohji Tomisaka, Chakali EswaraiahPatrick M. Koch, Kate Pattle, Chang Won Lee, Motohide Tamura, David Berry, Tao Chung Ching, Jihye Hwang, Woojin Kwon, Archana Soam, Jia Wei Wang, Shih Ping Lai, Keping Qiu, Derek Ward-Thompson, Do Young Byun, Huei Ru Vivien Chen, Wen Ping Chen, Zhiwei Chen, Jungyeon Cho, Minho Choi, Yunhee Choi, Antonio Chrysostomou, Eun Jung Chung, Pham Ngoc Diep, Hao Yuan Duan, Lapo Fanciullo, Jason Fiege, Erica Franzmann, Per Friberg, Gary Fuller, Tim Gledhill, Sarah F. Graves, Jane S. Greaves, Matt J. Griffin, Qilao Gu, Ilseung Han, Jennifer Hatchell, Saeko S. Hayashi, Thiem Hoang, Tsuyoshi Inoue, Kazunari Iwasaki, Il Gyo Jeong, Doug Johnstone, Yoshihiro Kanamori, Ji Hyun Kang, Miju Kang, Sung Ju Kang, Akimasa Kataoka, Koji S. Kawabata, Francisca Kemper, Gwanjeong Kim, Jongsoo Kim, Kee Tae Kim, Kyoung Hee Kim, Mi Ryang Kim, Shinyoung Kim, Jason M. Kirk, Masato I.N. Kobayashi, Vera Konyves, Takayoshi Kusune, Jungmi Kwon, Kevin Lacaille, Chi Yan Law, Chin Fei Lee, Hyeseung Lee, Jeong Eun Lee, Sang Sung Lee, Yong Hee Lee, Dalei Li, Di Li, Hua Bai Li, Hong Li Liu, Junhao Liu, Sheng Yuan Liu, Tie Liu, Ilse De Looze, A. Ran Lyo, Brenda C. Matthews, Gerald H. Moriarty-Schieven, Tetsuya Nagata, Fumitaka Nakamura, Hiroyuki Nakanishi, Nagayoshi Ohashi, Geumsook Park, Harriet Parsons, Nicolas Peretto, Tae Soo Pyo, Lei Qian, Ramprasad Rao, Mark G. Rawlings, Brendan Retter, John Richer, Andrew Rigby, Hiro Saito, Giorgio Savini, Anna M.M. Scaife, Masumichi Seta, Hiroko Shinnaga, Ya Wen Tang, Yusuke Tsukamoto, Serena Viti, Hongchi Wang, Anthony P. Whitworth, Hsi Wei Yen, Hyunju Yoo, Jinghua Yuan, Hyeong Sik Yun, Tetsuya Zenko, Chuan Peng Zhang, Guoyin Zhang, Yapeng Zhang, Jianjun Zhou, Lei Zhu, Philippe André, C. Darren Dowell, Stewart P.S. Eyres, Sam Falle, Sven Van Loo, Jean François Robitaille

Graduate Institute of Astronomy

Research output: Contribution to journal › Comment/debate

Abstract

In the published article, we presented high-resolution polarimetry data obtained by using JCMT SCUBA-2/POL-2, and compared them with the larger-scale magnetic structure observed by Planck (Planck Collaboration et al. 2020). There was a miscalculation in the analysis of the Planck data for comparison, and the mean position angle of the Planck magnetic field should be corrected from -40° ± 7° to -48° ± 6°. Thus, we replace the descriptions in the published article as follows. In Section 4.2, paragraph 3, the second sentence should read: "The differences between the orientations of IRAS 4A, IRAS 4B, and IRAS 2A are not statistically significant, but they do show significantly different orientations from those of the global B-field observed by Planck (-48° ± 6°; Section 4.1)." In Section 4.1, paragraph 3, the second line should read: "The Planck B-field orientation shows a smoothly and slowly varying field distribution with a position angle of -48° ± 6° in our observed NGC 1333 area." Accordingly, we replace Figures 4, 5, 9, 10, and 17 to reflect the correct Planck data. As described above, this error of modest magnitude is related only to our derivation of the Planck polarization angle, and the JCMT observation results are unaffected. Therefore, all conclusions drawn in the published article are unchanged even after the above correction is applied. The 1 pc scale magnetic field observed by Planck shows a smooth distribution, and the interstellar magnetic field in molecular clouds increases the complexity significantly on the scale of less than 1 pc.

Original language	English
Article number	abf2b3
Journal	Astrophysical Journal
Volume	911
Issue number	1
DOIs	https://doi.org/10.3847/1538-4357/abf2b3
State	Published - 16 Apr 2021

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10.3847/1538-4357/abf2b3

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Doi, Y., Hasegawa, T., Furuya, R. S., Coudé, S., Hull, C. L. H., Arzoumanian, D., Bastien, P., Chun-Yuan Chen, M., Di Francesco, J., Friesen, R., Houde, M., Inutsuka, S. I., Mairs, S., Matsumura, M., Onaka, T., Sadavoy, S., Shimajiri, Y., Tahani, M., Tomisaka, K., ... Robitaille, J. F. (2021). Erratum: The JCMT BISTRO survey: Magnetic fields associated with a network of filaments in NGC 1333 (Astrophysical Journal (2020) 899 (28) DOI: 10.3847/1538-4357/aba1e2). Astrophysical Journal, 911(1), Article abf2b3. https://doi.org/10.3847/1538-4357/abf2b3

@article{f0747c9db0e645a99fda25fe1405cb1f,

title = "Erratum: The JCMT BISTRO survey: Magnetic fields associated with a network of filaments in NGC 1333 (Astrophysical Journal (2020) 899 (28) DOI: 10.3847/1538-4357/aba1e2)",

abstract = "In the published article, we presented high-resolution polarimetry data obtained by using JCMT SCUBA-2/POL-2, and compared them with the larger-scale magnetic structure observed by Planck (Planck Collaboration et al. 2020). There was a miscalculation in the analysis of the Planck data for comparison, and the mean position angle of the Planck magnetic field should be corrected from -40° ± 7° to -48° ± 6°. Thus, we replace the descriptions in the published article as follows. In Section 4.2, paragraph 3, the second sentence should read: {"}The differences between the orientations of IRAS 4A, IRAS 4B, and IRAS 2A are not statistically significant, but they do show significantly different orientations from those of the global B-field observed by Planck (-48° ± 6°; Section 4.1).{"} In Section 4.1, paragraph 3, the second line should read: {"}The Planck B-field orientation shows a smoothly and slowly varying field distribution with a position angle of -48° ± 6° in our observed NGC 1333 area.{"} Accordingly, we replace Figures 4, 5, 9, 10, and 17 to reflect the correct Planck data. As described above, this error of modest magnitude is related only to our derivation of the Planck polarization angle, and the JCMT observation results are unaffected. Therefore, all conclusions drawn in the published article are unchanged even after the above correction is applied. The 1 pc scale magnetic field observed by Planck shows a smooth distribution, and the interstellar magnetic field in molecular clouds increases the complexity significantly on the scale of less than 1 pc.",

author = "Yasuo Doi and Tetsuo Hasegawa and Furuya, {Ray S.} and Simon Coud{\'e} and Hull, {Charles L.H.} and Doris Arzoumanian and Pierre Bastien and {Chun-Yuan Chen}, Michael and {Di Francesco}, James and Rachel Friesen and Martin Houde and Inutsuka, {Shu Ichiro} and Steve Mairs and Masafumi Matsumura and Takashi Onaka and Sarah Sadavoy and Yoshito Shimajiri and Mehrnoosh Tahani and Kohji Tomisaka and Chakali Eswaraiah and Koch, {Patrick M.} and Kate Pattle and Lee, {Chang Won} and Motohide Tamura and David Berry and Ching, {Tao Chung} and Jihye Hwang and Woojin Kwon and Archana Soam and Wang, {Jia Wei} and Lai, {Shih Ping} and Keping Qiu and Derek Ward-Thompson and Byun, {Do Young} and {Vivien Chen}, {Huei Ru} and Chen, {Wen Ping} and Zhiwei Chen and Jungyeon Cho and Minho Choi and Yunhee Choi and Antonio Chrysostomou and Chung, {Eun Jung} and Diep, {Pham Ngoc} and Duan, {Hao Yuan} and Lapo Fanciullo and Jason Fiege and Erica Franzmann and Per Friberg and Gary Fuller and Tim Gledhill and Graves, {Sarah F.} and Greaves, {Jane S.} and Griffin, {Matt J.} and Qilao Gu and Ilseung Han and Jennifer Hatchell and Hayashi, {Saeko S.} and Thiem Hoang and Tsuyoshi Inoue and Kazunari Iwasaki and Jeong, {Il Gyo} and Doug Johnstone and Yoshihiro Kanamori and Kang, {Ji Hyun} and Miju Kang and Kang, {Sung Ju} and Akimasa Kataoka and Kawabata, {Koji S.} and Francisca Kemper and Gwanjeong Kim and Jongsoo Kim and Kim, {Kee Tae} and Kim, {Kyoung Hee} and Kim, {Mi Ryang} and Shinyoung Kim and Kirk, {Jason M.} and Kobayashi, {Masato I.N.} and Vera Konyves and Takayoshi Kusune and Jungmi Kwon and Kevin Lacaille and Law, {Chi Yan} and Lee, {Chin Fei} and Hyeseung Lee and Lee, {Jeong Eun} and Lee, {Sang Sung} and Lee, {Yong Hee} and Dalei Li and Di Li and Li, {Hua Bai} and Liu, {Hong Li} and Junhao Liu and Liu, {Sheng Yuan} and Tie Liu and {De Looze}, Ilse and Lyo, {A. Ran} and Matthews, {Brenda C.} and Moriarty-Schieven, {Gerald H.} and Tetsuya Nagata and Fumitaka Nakamura and Hiroyuki Nakanishi and Nagayoshi Ohashi and Geumsook Park and Harriet Parsons and Nicolas Peretto and Pyo, {Tae Soo} and Lei Qian and Ramprasad Rao and Rawlings, {Mark G.} and Brendan Retter and John Richer and Andrew Rigby and Hiro Saito and Giorgio Savini and Scaife, {Anna M.M.} and Masumichi Seta and Hiroko Shinnaga and Tang, {Ya Wen} and Yusuke Tsukamoto and Serena Viti and Hongchi Wang and Whitworth, {Anthony P.} and Yen, {Hsi Wei} and Hyunju Yoo and Jinghua Yuan and Yun, {Hyeong Sik} and Tetsuya Zenko and Zhang, {Chuan Peng} and Guoyin Zhang and Yapeng Zhang and Jianjun Zhou and Lei Zhu and Philippe Andr{\'e} and {Darren Dowell}, C. and Eyres, {Stewart P.S.} and Sam Falle and {Van Loo}, Sven and Robitaille, {Jean Fran{\c c}ois}",

year = "2021",

month = apr,

day = "16",

doi = "10.3847/1538-4357/abf2b3",

language = "???core.languages.en_GB???",

volume = "911",

journal = "Astrophysical Journal",

issn = "0004-637X",

number = "1",

}

Doi, Y, Hasegawa, T, Furuya, RS, Coudé, S, Hull, CLH, Arzoumanian, D, Bastien, P, Chun-Yuan Chen, M, Di Francesco, J, Friesen, R, Houde, M, Inutsuka, SI, Mairs, S, Matsumura, M, Onaka, T, Sadavoy, S, Shimajiri, Y, Tahani, M, Tomisaka, K, Eswaraiah, C, Koch, PM, Pattle, K, Lee, CW, Tamura, M, Berry, D, Ching, TC, Hwang, J, Kwon, W, Soam, A, Wang, JW, Lai, SP, Qiu, K, Ward-Thompson, D, Byun, DY, Vivien Chen, HR, Chen, WP, Chen, Z, Cho, J, Choi, M, Choi, Y, Chrysostomou, A, Chung, EJ, Diep, PN, Duan, HY, Fanciullo, L, Fiege, J, Franzmann, E, Friberg, P, Fuller, G, Gledhill, T, Graves, SF, Greaves, JS, Griffin, MJ, Gu, Q, Han, I, Hatchell, J, Hayashi, SS, Hoang, T, Inoue, T, Iwasaki, K, Jeong, IG, Johnstone, D, Kanamori, Y, Kang, JH, Kang, M, Kang, SJ, Kataoka, A, Kawabata, KS, Kemper, F, Kim, G, Kim, J, Kim, KT, Kim, KH, Kim, MR, Kim, S, Kirk, JM, Kobayashi, MIN, Konyves, V, Kusune, T, Kwon, J, Lacaille, K, Law, CY, Lee, CF, Lee, H, Lee, JE, Lee, SS, Lee, YH, Li, D, Li, D, Li, HB, Liu, HL, Liu, J, Liu, SY, Liu, T, De Looze, I, Lyo, AR, Matthews, BC, Moriarty-Schieven, GH, Nagata, T, Nakamura, F, Nakanishi, H, Ohashi, N, Park, G, Parsons, H, Peretto, N, Pyo, TS, Qian, L, Rao, R, Rawlings, MG, Retter, B, Richer, J, Rigby, A, Saito, H, Savini, G, Scaife, AMM, Seta, M, Shinnaga, H, Tang, YW, Tsukamoto, Y, Viti, S, Wang, H, Whitworth, AP, Yen, HW, Yoo, H, Yuan, J, Yun, HS, Zenko, T, Zhang, CP, Zhang, G, Zhang, Y, Zhou, J, Zhu, L, André, P, Darren Dowell, C, Eyres, SPS, Falle, S, Van Loo, S & Robitaille, JF 2021, 'Erratum: The JCMT BISTRO survey: Magnetic fields associated with a network of filaments in NGC 1333 (Astrophysical Journal (2020) 899 (28) DOI: 10.3847/1538-4357/aba1e2)', Astrophysical Journal, vol. 911, no. 1, abf2b3. https://doi.org/10.3847/1538-4357/abf2b3

TY - JOUR

T1 - Erratum

T2 - The JCMT BISTRO survey: Magnetic fields associated with a network of filaments in NGC 1333 (Astrophysical Journal (2020) 899 (28) DOI: 10.3847/1538-4357/aba1e2)

AU - Doi, Yasuo

AU - Hasegawa, Tetsuo

AU - Furuya, Ray S.

AU - Coudé, Simon

AU - Hull, Charles L.H.

AU - Arzoumanian, Doris

AU - Bastien, Pierre

AU - Chun-Yuan Chen, Michael

AU - Di Francesco, James

AU - Friesen, Rachel

AU - Houde, Martin

AU - Inutsuka, Shu Ichiro

AU - Mairs, Steve

AU - Matsumura, Masafumi

AU - Onaka, Takashi

AU - Sadavoy, Sarah

AU - Shimajiri, Yoshito

AU - Tahani, Mehrnoosh

AU - Tomisaka, Kohji

AU - Eswaraiah, Chakali

AU - Koch, Patrick M.

AU - Pattle, Kate

AU - Lee, Chang Won

AU - Tamura, Motohide

AU - Berry, David

AU - Ching, Tao Chung

AU - Hwang, Jihye

AU - Kwon, Woojin

AU - Soam, Archana

AU - Wang, Jia Wei

AU - Lai, Shih Ping

AU - Qiu, Keping

AU - Ward-Thompson, Derek

AU - Byun, Do Young

AU - Vivien Chen, Huei Ru

AU - Chen, Wen Ping

AU - Chen, Zhiwei

AU - Cho, Jungyeon

AU - Choi, Minho

AU - Choi, Yunhee

AU - Chrysostomou, Antonio

AU - Chung, Eun Jung

AU - Diep, Pham Ngoc

AU - Duan, Hao Yuan

AU - Fanciullo, Lapo

AU - Fiege, Jason

AU - Franzmann, Erica

AU - Friberg, Per

AU - Fuller, Gary

AU - Gledhill, Tim

AU - Graves, Sarah F.

AU - Greaves, Jane S.

AU - Griffin, Matt J.

AU - Gu, Qilao

AU - Han, Ilseung

AU - Hatchell, Jennifer

AU - Hayashi, Saeko S.

AU - Hoang, Thiem

AU - Inoue, Tsuyoshi

AU - Iwasaki, Kazunari

AU - Jeong, Il Gyo

AU - Johnstone, Doug

AU - Kanamori, Yoshihiro

AU - Kang, Ji Hyun

AU - Kang, Miju

AU - Kang, Sung Ju

AU - Kataoka, Akimasa

AU - Kawabata, Koji S.

AU - Kemper, Francisca

AU - Kim, Gwanjeong

AU - Kim, Jongsoo

AU - Kim, Kee Tae

AU - Kim, Kyoung Hee

AU - Kim, Mi Ryang

AU - Kim, Shinyoung

AU - Kirk, Jason M.

AU - Kobayashi, Masato I.N.

AU - Konyves, Vera

AU - Kusune, Takayoshi

AU - Kwon, Jungmi

AU - Lacaille, Kevin

AU - Law, Chi Yan

AU - Lee, Chin Fei

AU - Lee, Hyeseung

AU - Lee, Jeong Eun

AU - Lee, Sang Sung

AU - Lee, Yong Hee

AU - Li, Dalei

AU - Li, Di

AU - Li, Hua Bai

AU - Liu, Hong Li

AU - Liu, Junhao

AU - Liu, Sheng Yuan

AU - Liu, Tie

AU - De Looze, Ilse

AU - Lyo, A. Ran

AU - Matthews, Brenda C.

AU - Moriarty-Schieven, Gerald H.

AU - Nagata, Tetsuya

AU - Nakamura, Fumitaka

AU - Nakanishi, Hiroyuki

AU - Ohashi, Nagayoshi

AU - Park, Geumsook

AU - Parsons, Harriet

AU - Peretto, Nicolas

AU - Pyo, Tae Soo

AU - Qian, Lei

AU - Rao, Ramprasad

AU - Rawlings, Mark G.

AU - Retter, Brendan

AU - Richer, John

AU - Rigby, Andrew

AU - Saito, Hiro

AU - Savini, Giorgio

AU - Scaife, Anna M.M.

AU - Seta, Masumichi

AU - Shinnaga, Hiroko

AU - Tang, Ya Wen

AU - Tsukamoto, Yusuke

AU - Viti, Serena

AU - Wang, Hongchi

AU - Whitworth, Anthony P.

AU - Yen, Hsi Wei

AU - Yoo, Hyunju

AU - Yuan, Jinghua

AU - Yun, Hyeong Sik

AU - Zenko, Tetsuya

AU - Zhang, Chuan Peng

AU - Zhang, Guoyin

AU - Zhang, Yapeng

AU - Zhou, Jianjun

AU - Zhu, Lei

AU - André, Philippe

AU - Darren Dowell, C.

AU - Eyres, Stewart P.S.

AU - Falle, Sam

AU - Van Loo, Sven

AU - Robitaille, Jean François

PY - 2021/4/16

Y1 - 2021/4/16

N2 - In the published article, we presented high-resolution polarimetry data obtained by using JCMT SCUBA-2/POL-2, and compared them with the larger-scale magnetic structure observed by Planck (Planck Collaboration et al. 2020). There was a miscalculation in the analysis of the Planck data for comparison, and the mean position angle of the Planck magnetic field should be corrected from -40° ± 7° to -48° ± 6°. Thus, we replace the descriptions in the published article as follows. In Section 4.2, paragraph 3, the second sentence should read: "The differences between the orientations of IRAS 4A, IRAS 4B, and IRAS 2A are not statistically significant, but they do show significantly different orientations from those of the global B-field observed by Planck (-48° ± 6°; Section 4.1)." In Section 4.1, paragraph 3, the second line should read: "The Planck B-field orientation shows a smoothly and slowly varying field distribution with a position angle of -48° ± 6° in our observed NGC 1333 area." Accordingly, we replace Figures 4, 5, 9, 10, and 17 to reflect the correct Planck data. As described above, this error of modest magnitude is related only to our derivation of the Planck polarization angle, and the JCMT observation results are unaffected. Therefore, all conclusions drawn in the published article are unchanged even after the above correction is applied. The 1 pc scale magnetic field observed by Planck shows a smooth distribution, and the interstellar magnetic field in molecular clouds increases the complexity significantly on the scale of less than 1 pc.

AB - In the published article, we presented high-resolution polarimetry data obtained by using JCMT SCUBA-2/POL-2, and compared them with the larger-scale magnetic structure observed by Planck (Planck Collaboration et al. 2020). There was a miscalculation in the analysis of the Planck data for comparison, and the mean position angle of the Planck magnetic field should be corrected from -40° ± 7° to -48° ± 6°. Thus, we replace the descriptions in the published article as follows. In Section 4.2, paragraph 3, the second sentence should read: "The differences between the orientations of IRAS 4A, IRAS 4B, and IRAS 2A are not statistically significant, but they do show significantly different orientations from those of the global B-field observed by Planck (-48° ± 6°; Section 4.1)." In Section 4.1, paragraph 3, the second line should read: "The Planck B-field orientation shows a smoothly and slowly varying field distribution with a position angle of -48° ± 6° in our observed NGC 1333 area." Accordingly, we replace Figures 4, 5, 9, 10, and 17 to reflect the correct Planck data. As described above, this error of modest magnitude is related only to our derivation of the Planck polarization angle, and the JCMT observation results are unaffected. Therefore, all conclusions drawn in the published article are unchanged even after the above correction is applied. The 1 pc scale magnetic field observed by Planck shows a smooth distribution, and the interstellar magnetic field in molecular clouds increases the complexity significantly on the scale of less than 1 pc.

UR - http://www.scopus.com/inward/record.url?scp=85105607212&partnerID=8YFLogxK

U2 - 10.3847/1538-4357/abf2b3

DO - 10.3847/1538-4357/abf2b3

M3 - 評論/辯論

AN - SCOPUS:85105607212

SN - 0004-637X

VL - 911

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 1

M1 - abf2b3

ER -

Erratum: The JCMT BISTRO survey: Magnetic fields associated with a network of filaments in NGC 1333 (Astrophysical Journal (2020) 899 (28) DOI: 10.3847/1538-4357/aba1e2)

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